Adiabatic processes
Storyboard 
In processes that occur rapidly, there is not enough time for the internal energy to vary significantly. In this case, any work done reduces the heat of the system, leading to modifications in the ideal gas equations.
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Mechanisms
Definition 
An adiabatic process is a thermodynamic process in which no heat is exchanged between the system and its surroundings. This means that all changes in the system's internal energy result solely from work done on or by the system. In an adiabatic expansion, the system does work on its surroundings, causing its temperature to drop. Conversely, in an adiabatic compression, work is done on the system, increasing its temperature. These processes are often idealized and occur in well-insulated systems where heat transfer is negligible.
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Adiabatic process
Image 
When a gas expands rapidly, the water vapor molecules do not have enough time to exchange energy with the surroundings, so no heat is transferred, that is, the variation of heat ($\delta Q$) remains constant:
$\delta Q = 0$
The processes that are carried out under this condition are called adiabatic processes [1,2].
The expansion of the gas requires the system to do work or generate the differential inexact labour ($\delta W$). However, the energy needed for this cannot come from the internal energy ($U$), so it must be obtained from heat. As a result, the temperature of the system decreases, leading to a decrease in the variation of heat ($\delta Q$).
A typical example of this process is the formation of clouds. When air rises through convection, it expands, performs work, and cools down. The moisture in the air condenses, forming clouds.
Conversely, when work is done on the system, positive work the differential inexact labour ($\delta W$) is done. However, since the internal energy ($U$) cannot increase, the thermal energy in the variation of heat ($\delta Q$) increases, leading to an increase in the system's temperature.
A common example of this process is using a pump. If we try to inflate something rapidly, we do work on the system adiabatically, leading to an increase in ERROR:5202
[1] "Réflexions sur la puissance motrice du feu" (Reflections on the Motive Power of Fire), Sadi Carnot, 1824
[2] "Über die bewegende Kraft der Wärme und die Gesetze, welche sich daraus für die Wärmelehre selbst ableiten lassen" (On the Moving Force of Heat and the Laws Which Can Be Deduced from It for the Theory of Heat Itself), Rudolf Clausius, Annalen der Physik und Chemie, 1850
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First law of Thermodynamics and Pressure
Note 
Since the internal energy differential ($dU$) relates to the differential inexact Heat ($\delta Q$) and the differential inexact labour ($\delta W$) as shown below:
| $ dU = \delta Q - \delta W $ |
And it is known that the differential inexact labour ($\delta W$) is related to the pressure ($p$) and the volume Variation ($\Delta V$) as follows:
| $ \delta W = p dV $ |
Therefore, we can conclude that:
| $ dU = \delta Q - p dV $ |
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Caloric content of a gas at constant volume as a function of specific heat
Quote 
The variation of the internal energy ($dU$) in relation to the temperature variation ($\Delta T$) and the heat capacity at constant volume ($C_V$) is expressed as:
| $ dU = C_V \Delta T $ |
Where the heat capacity at constant volume ($C_V$) can be replaced by the specific heat of gases at constant volume ($c_V$) and the mass ($M$) using the following relationship:
| $ c_V =\displaystyle\frac{ C_V }{ M }$ |
Therefore, we obtain:
| $ dU = c_V m \Delta T $ |
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Temperature and Volume Variation
Exercise 
Since with the variation of the internal energy ($dU$), the variation of heat ($\delta Q$), and the differential inexact labour ($\delta W$) we have:
$dU = \delta Q - \delta W = 0 - \delta W = - \delta W$
the variation of the internal energy ($dU$) can be calculated from the specific heat of gases at constant volume ($c_V$), the mass ($M$) and the temperature variation ($\Delta T$) in the case of a constant volume:
| $ dU = c_V m \Delta T $ |
Similarly, we can replace the differential inexact labour ($\delta W$) with the pressure ($p$) and the volume Variation ($\Delta V$):
| $ \delta W = p dV $ |
If we equate both expressions, we obtain the equation:
$c_VMdT=-pdV$
Which, with the inclusion of the volume ($V$), the universal gas constant ($R_C$), and ERROR:6679, leads to:
| $ p V = n R_C T $ |
And with the mass ($M$) and the molar Mass ($M_m$):
| $ n = \displaystyle\frac{ M }{ M_m }$ |
Finally, in the limit $\Delta T \rightarrow dt$, we obtain the relationship:
| $\displaystyle\frac{ dT }{ T }=-\displaystyle\frac{ R_C }{ M_m c_V }\displaystyle\frac{ dV }{ V }$ |
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Adiabatic case relationship of temperature and volume
Equation 
In the adiabatic case, for ERROR:5177,0 and the volume ($V$) with the universal gas constant ($R_C$), the molar Mass ($M_m$), the specific heat of gases at constant volume ($c_V$), the temperature variation ($dT$), and the volume Variation ($\Delta V$), we have the following equation:
| $\displaystyle\frac{ dT }{ T }=-\displaystyle\frac{ R_C }{ M_m c_V }\displaystyle\frac{ dV }{ V }$ |
By introducing the adiabatic index ($\kappa$), this equation can be expressed as:
| $ \kappa \equiv1+\displaystyle\frac{ R_C }{ M_m c_V }$ |
This allows us to write the equation as:
$\displaystyle\frac{dT}{T}=-(\kappa - 1)\displaystyle\frac{dV}{V}$
If we integrate this expression between the volume in state i ($V_i$) and the volume in state f ($V_f$), as well as between the temperature in initial state ($T_i$) and the temperature in final state ($T_f$), we obtain:
| $ T_i V_i ^{ \kappa -1}= T_f V_f ^{ \kappa -1}$ |
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Adiabatic processes
Description 
An adiabatic process is a thermodynamic process in which no heat is exchanged between the system and its surroundings. This means that all changes in the system's internal energy result solely from work done on or by the system. In an adiabatic expansion, the system does work on its surroundings, causing its temperature to drop. Conversely, in an adiabatic compression, work is done on the system, increasing its temperature. These processes are often idealized and occur in well-insulated systems where heat transfer is negligible.
Variables
Calculations
Calculations
Equations
The pressure ($p$), the volume ($V$), the absolute temperature ($T$), and the number of moles ($n$) are related through the following physical laws:
• Boyle's law
| $ p V = C_b $ |
• Charles's law
| $\displaystyle\frac{ V }{ T } = C_c$ |
• Gay-Lussac's law
| $\displaystyle\frac{ p }{ T } = C_g$ |
• Avogadro's law
| $\displaystyle\frac{ n }{ V } = C_a $ |
These laws can be expressed in a more general form as:
$\displaystyle\frac{pV}{nT}=cte$
This general relationship states that the product of pressure and volume divided by the number of moles and temperature remains constant:
| $ p V = n R_C T $ |
(ID 3183)
The pressure ($p$), the volume ($V$), the absolute temperature ($T$), and the number of moles ($n$) are related through the following physical laws:
• Boyle's law
| $ p V = C_b $ |
• Charles's law
| $\displaystyle\frac{ V }{ T } = C_c$ |
• Gay-Lussac's law
| $\displaystyle\frac{ p }{ T } = C_g$ |
• Avogadro's law
| $\displaystyle\frac{ n }{ V } = C_a $ |
These laws can be expressed in a more general form as:
$\displaystyle\frac{pV}{nT}=cte$
This general relationship states that the product of pressure and volume divided by the number of moles and temperature remains constant:
| $ p V = n R_C T $ |
(ID 3183)
(ID 4381)
(ID 4860)
In the adiabatic case, for ERROR:5177,0 and the volume ($V$) with the universal gas constant ($R_C$), the molar Mass ($M_m$), the specific heat at constant pressure ($c_p$), the temperature variation ($dT$), and the volume Variation ($\Delta V$), we have the following equation:
| $\displaystyle\frac{ dT }{ T }=-\displaystyle\frac{ R_C }{ M_m c_V }\displaystyle\frac{ dV }{ V }$ |
By introducing the adiabatic index ($\kappa$), this equation can be expressed as:
| $ \kappa \equiv1+\displaystyle\frac{ R_C }{ M_m c_V }$ |
This allows us to write the equation as:
$\displaystyle\frac{dT}{T}=-(\kappa - 1)\displaystyle\frac{dV}{V}$
If we integrate this expression between the volume in state i ($V_i$) and the volume in state f ($V_f$), as well as between the temperature in initial state ($T_i$) and the temperature in final state ($T_f$), we obtain:
| $ T_i V_i ^{ \kappa -1}= T_f V_f ^{ \kappa -1}$ |
(ID 4865)
The variation of the internal energy ($dU$) in relation to the temperature variation ($\Delta T$) and the heat capacity at constant volume ($C_V$) is expressed as:
| $ dU = C_V \Delta T $ |
Where the heat capacity at constant volume ($C_V$) can be replaced by the specific heat of gases at constant volume ($c_V$) and the mass ($M$) using the following relationship:
| $ c_V =\displaystyle\frac{ C_V }{ M }$ |
Therefore, we obtain:
| $ dU = c_V M \Delta T $ |
(ID 11115)
Examples
An adiabatic change in a gas occurs when the process is so rapid that there is no time for the system to exchange heat with the surrounding medium. A classic example is the ascent of an air mass in the atmosphere: as it rises to a region of lower pressure and does not interact thermally with its environment, the gas expands. This expansion requires mechanical work, which is performed at the expense of the gas's internal energy, resulting in a decrease in temperature. This final temperature usually differs from the ambient temperature.
The temperature after such a change can be calculated using the adiabatic relations. Once the change occurs, if there is a temperature difference between the gas and the environment, heat exchange begins: the gas absorbs heat if its temperature is lower than the mediums, or releases heat if it is higher. In this stage, the adiabatic equations are no longer valid, and the system evolves toward thermal equilibrium.
You can explore this behavior with the following simulator. Set the initial pressure and temperature of the gas, and the pressure and temperature of the surrounding medium. The simulator will first show the adiabatic change ($\delta Q=0$), followed by the thermal evolution as the gas exchanges heat. The graph shows the heat absorbed (positive) or released (negative):
You may also experiment with different gases by adjusting $\kappa$ (the heat capacity ratio), the molar heat capacity (default: 20.79 J/mol K), and the thermal conductivity (default: 1 J/K), using values that are physically realistic or atmospheric.
Note that the ideal gas law (relating pressure $p$, volume $V$, and temperature $T$) always holds. A sudden change in pressure modifies only one of these variables, so an additional equation is needed. In adiabatic conditions, this is provided by the first law of thermodynamics, which simplifies to a relation between $V$ and $T$ when no heat is exchanged. Once heat exchange begins, the process is no longer adiabatic, but the ideal gas law remains valid. The adiabatic equations do not contradict the gas laws; they provide extra constraints that fully determine the system during the rapid transition.
(ID 15262)
When a gas expands rapidly, the water vapor molecules do not have enough time to exchange energy with the surroundings, so no heat is transferred, that is, the variation of heat ($\delta Q$) remains constant:
$\delta Q = 0$
The processes that are carried out under this condition are called adiabatic processes [1,2].
The expansion of the gas requires the system to do work or generate the differential inexact labour ($\delta W$). However, the energy needed for this cannot come from the internal energy ($U$), so it must be obtained from heat. As a result, the temperature of the system decreases, leading to a decrease in the variation of heat ($\delta Q$).
A typical example of this process is the formation of clouds. When air rises through convection, it expands, performs work, and cools down. The moisture in the air condenses, forming clouds.
Conversely, when work is done on the system, positive work the differential inexact labour ($\delta W$) is done. However, since the internal energy ($U$) cannot increase, the thermal energy in the variation of heat ($\delta Q$) increases, leading to an increase in the system's temperature.
A common example of this process is using a pump. If we try to inflate something rapidly, we do work on the system adiabatically, leading to an increase in ERROR:5202
[1] "R flexions sur la puissance motrice du feu" (Reflections on the Motive Power of Fire), Sadi Carnot, 1824
[2] " ber die bewegende Kraft der W rme und die Gesetze, welche sich daraus f r die W rmelehre selbst ableiten lassen" (On the Moving Force of Heat and the Laws Which Can Be Deduced from It for the Theory of Heat Itself), Rudolf Clausius, Annalen der Physik und Chemie, 1850
(ID 41)
The variation of the internal energy ($dU$) in relation to the temperature variation ($\Delta T$) and the heat capacity at constant volume ($C_V$) is expressed as:
| $ dU = C_V \Delta T $ |
Where the heat capacity at constant volume ($C_V$) can be replaced by the specific heat of gases at constant volume ($c_V$) and the mass ($M$) using the following relationship:
| $ c_V =\displaystyle\frac{ C_V }{ M }$ |
Therefore, we obtain:
| $ dU = c_V m \Delta T $ |
(ID 15739)
Since with the variation of the internal energy ($dU$), the variation of heat ($\delta Q$), and the differential inexact labour ($\delta W$) we have:
$dU = \delta Q - \delta W = 0 - \delta W = - \delta W$
the variation of the internal energy ($dU$) can be calculated from the specific heat of gases at constant volume ($c_V$), the mass ($M$) and the temperature variation ($\Delta T$) in the case of a constant volume:
| $ dU = c_V m \Delta T $ |
Similarly, we can replace the differential inexact labour ($\delta W$) with the pressure ($p$) and the volume Variation ($\Delta V$):
| $ \delta W = p dV $ |
If we equate both expressions, we obtain the equation:
$c_VMdT=-pdV$
Which, with the inclusion of the volume ($V$), the universal gas constant ($R_C$), and ERROR:6679, leads to:
| $ p V = n R_C T $ |
And with the mass ($M$) and the molar Mass ($M_m$):
| $ n = \displaystyle\frac{ M }{ M_m }$ |
Finally, in the limit $\Delta T \rightarrow dt$, we obtain the relationship:
| $\displaystyle\frac{ dT }{ T }=-\displaystyle\frac{ R_C }{ M_m c_V }\displaystyle\frac{ dV }{ V }$ |
(ID 15740)
In the adiabatic case, for the absolute temperature ($T$) and the volume ($V$) with the universal gas constant ($R_C$), the molar Mass ($M_m$), the specific heat of gases at constant volume ($c_V$), the temperature variation ($dT$), and the volume Variation ($\Delta V$), we have the following equation:
| $\displaystyle\frac{ dT }{ T }=-\displaystyle\frac{ R_C }{ M_m c_V }\displaystyle\frac{ dV }{ V }$ |
By introducing the adiabatic index ($\kappa$), this equation can be expressed as:
| $ \kappa \equiv1+\displaystyle\frac{ R_C }{ M_m c_V }$ |
This allows us to write the equation as:
$\displaystyle\frac{dT}{T}=-(\kappa - 1)\displaystyle\frac{dV}{V}$
If we integrate this expression between the volume in state i ($V_i$) and the volume in state f ($V_f$), as well as between the temperature in initial state ($T_i$) and the temperature in final state ($T_f$), we obtain:
| $ T_i V_i ^{ \kappa -1}= T_f V_f ^{ \kappa -1}$ |
(ID 15741)
(ID 15321)
In the adiabatic case, the system does not have the ability to alter the caloric Content ($Q$), meaning that the differential inexact Heat ($\delta Q$) must be zero:
| $ \delta Q =0$ |
(ID 4860)
The internal energy differential ($dU$) is always equal to the amount of the differential inexact Heat ($\delta Q$) supplied to the system (positive) minus the amount of the differential inexact labour ($\delta W$) performed by the system (negative):
| $ dU = \delta Q - \delta W $ |
(ID 9632)
The relationship between the variation of the variation of the internal energy ($dU$) and the temperature variation ($\Delta T$) is with the specific heat of gases at constant volume ($c_V$) and the mass ($M$) equal to:
| $ dU = c_V M \Delta T $ |
(ID 11115)
If a system is initially at ERROR:5236.1 and then is at the temperature in final state ($T_f$), the difference will be:
| $ \Delta T = T_f- T_i$ |
The temperature difference is independent of whether these values are in degrees Celsius or Kelvin.
(ID 4381)
The particle mass ($m$) can be estimated from the molar Mass ($M_m$) and the avogadro's number ($N_A$) using
| $ m =\displaystyle\frac{ M_m }{ N_A }$ |
(ID 4389)
Using the universal gas constant ($R_C$), the molar Mass ($M_m$), the specific heat of gases at constant volume ($c_V$), the temperature variation ($dT$), and the volume Variation ($\Delta V$), the adiabatic index ($\kappa$) can be defined as follows:
| $ \kappa \equiv1+\displaystyle\frac{ R_C }{ M_m c_V }$ |
(ID 4864)
In the case of an adiabatic process, the work in an Adiabatic Process ($\Delta W$) can be calculated from the values of the pressure in initial state ($p_i$), the volume in state i ($V_i$), the pressure in final state ($p_f$), the volume in state f ($V_f$), and the adiabatic index ($\kappa$), according to the following expression:
| $ \Delta W = \displaystyle\frac{ p_i V_i - p_f V_f }{ \kappa - 1}$ |
(ID 16222)
The pressure ($p$), the volume ($V$), the absolute temperature ($T$), and the number of moles ($n$) are related by the following equation:
| $ p V = n R_C T $ |
where the universal gas constant ($R_C$) has a value of 8.314 J/K mol.
(ID 3183)
The pressure ($p$), the volume ($V$), the absolute temperature ($T$), and the number of moles ($n$) are related by the following equation:
| $ p V = n R_C T $ |
where the universal gas constant ($R_C$) has a value of 8.314 J/K mol.
(ID 3183)
The pressure in initial state ($p_i$), the volume in state i ($V_i$), the temperature in initial state ($T_i$), the pressure in final state ($p_f$), the volume in state f ($V_f$), and the temperature in final state ($T_f$) are related by the following equation:
| $ \displaystyle\frac{ p_i V_i }{ T_i } = \displaystyle\frac{ p_f V_f }{ T_f }$ |
(ID 16221)
From an initial state (i) with the volume in state i ($V_i$) and the temperature in initial state ($T_i$) it goes to a final state (f) with the volume in state f ($V_f$) and the temperature in final state ($T_f$) according to:
| $ T_i V_i ^{ \kappa -1}= T_f V_f ^{ \kappa -1}$ |
(ID 4865)
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